The first stars: formation, properties, and impact

RS Klessen, SCO Glover - Annual Review of Astronomy and …, 2023 - annualreviews.org
The first generation of stars, often called Population III (or Pop III), form from metal-free
primordial gas at redshifts z∼ 30 and below. They dominate the cosmic star-formation …

Astrophysics with the laser interferometer space antenna

P Amaro-Seoane, J Andrews, M Arca Sedda… - Living Reviews in …, 2023 - Springer
Abstract The Laser Interferometer Space Antenna (LISA) will be a transformative experiment
for gravitational wave astronomy, and, as such, it will offer unique opportunities to address …

The origins of massive black holes

M Volonteri, M Habouzit, M Colpi - Nature Reviews Physics, 2021 - nature.com
Massive black holes (MBHs) inhabit galactic centres, and power luminous quasars and
active galactic nuclei, shaping their cosmic environment with the energy they produce. The …

The assembly of the first massive black holes

K Inayoshi, E Visbal, Z Haiman - Annual Review of Astronomy …, 2020 - annualreviews.org
The existence of∼ 109M⊙ supermassive black holes (SMBHs) within the first billion years
of the Universe has stimulated numerous ideas for the prompt formation and rapid growth of …

What if young z > 9 JWST galaxies hosted massive black holes?

M Volonteri, M Habouzit, M Colpi - Monthly Notices of the Royal …, 2023 - academic.oup.com
ABSTRACT JWST is discovering star-forming 'candidate'galaxies with photometric redshifts
z> 9 and little attenuation. We model presumptive massive black holes (MBHs) in such …

Formation of black holes in the pair-instability mass gap: evolution of a post-collision star

G Costa, A Ballone, M Mapelli… - Monthly Notices of the …, 2022 - academic.oup.com
The detection of GW190521 by the LIGO–Virgo collaboration has revealed the existence of
black holes (BHs) in the pair-instability (PI) mass gap. Here, we investigate the formation of …

Formation sites of Population III star formation: The effects of different levels of rotation and turbulence on the fragmentation behaviour of primordial gas

KMJ Wollenberg, SCO Glover, PC Clark… - Monthly Notices of the …, 2020 - academic.oup.com
We use the moving-mesh code arepo to investigate the effects of different levels of rotation
and turbulence on the fragmentation of primordial gas and the formation of Population III …

Supermassive star formation via super competitive accretion in slightly metal-enriched clouds

S Chon, K Omukai - Monthly Notices of the Royal Astronomical …, 2020 - academic.oup.com
Direct collapse black hole (DCBH) formation with mass≳ 105 M⊙ is a promising scenario
for the origin of high-redshift supermassive black holes. It has usually been supposed that …

The search for the farthest quasar: consequences for black hole growth and seed models

F Pacucci, A Loeb - Monthly Notices of the Royal Astronomical …, 2022 - academic.oup.com
The quest for high-redshift quasars has led to a series of record-breaking sources, with the
current record holder at z= 7.642. Here, we show how future detections of z> 8 quasars …

Origin of supermassive black holes in massive metal-poor protoclusters

DRG Schleicher, B Reinoso, M Latif… - Monthly Notices of …, 2022 - academic.oup.com
While large numbers of supermassive black holes have been detected at z> 6, their origin is
still essentially unclear. Numerical simulations have shown that the conditions for the …